Low-energy reaction yields for O18(p,γ) and O18(α,γ)

R. B. Vogelaar, T. R. Wang, S. E. Kellogg, and R. W. Kavanagh
Phys. Rev. C 42, 753 – Published 1 August 1990
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Abstract

Resonance yields, γ-ray branching, and low-energy limits have been measured for O18(p,γ) and O18(α,γ), for Ep<0.22 MeV and Eα<0.78 MeV, using a 4π array of NaI detectors. The results confirm previous resonance strengths, and set additional constraints on possible low-energy contributions to stellar reaction rates.

  • Received 16 October 1989

DOI:https://doi.org/10.1103/PhysRevC.42.753

©1990 American Physical Society

Authors & Affiliations

R. B. Vogelaar, T. R. Wang, S. E. Kellogg, and R. W. Kavanagh

  • W. K. Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, California 91125

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Vol. 42, Iss. 2 — August 1990

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